Surface-accretion disk models with fragile icy dust produce order-of-magnitude higher inner-disk water vapor enrichment and an anti-correlation between vapor concentration and residual gas mass.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Heavy element enrichment of gas in surface-accretion disks: A possible origin of the mass-metallicity anti-correlation in exoplanets
Surface-accretion disk models with fragile icy dust produce order-of-magnitude higher inner-disk water vapor enrichment and an anti-correlation between vapor concentration and residual gas mass.